| dc.contributor.author | An, Fang Xia | |
| dc.contributor.author | Smail, Ian | |
| dc.contributor.author | Swinbank, A. M. | |
| dc.date.accessioned | 2021-02-08T12:59:33Z | |
| dc.date.available | 2021-02-08T12:59:33Z | |
| dc.date.issued | 2020 | |
| dc.identifier.citation | An, F. X. et al. (2020). An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 sub-millimetre galaxies. Monthly Notices of the Royal Astronomical Society, 494(3), 3828–3860 | en_US |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/staa769 | |
| dc.identifier.uri | http://hdl.handle.net/10566/5867 | |
| dc.description.abstract | We analyse the physical properties of a large, homogeneously selected sample of ALMA-located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across the ∼1 deg2 field, including ∼17 per cent, which are undetected at K ≳ 25.7 mag. We interpret their ultraviolet-to-radio data using MAGPHYS and determine a median redshift of z = 2.61 ± 0.08 (1σ range of z = 1.8–3.4) with just ∼6 per cent at z > 4. Our survey provides a sample of massive dusty galaxies at z ≳ 1, with median dust and stellar masses of Md = (6.8 ± 0.3) × 108 M⊙ (thus, gas masses of ∼1011 M⊙) and M* = (1.26 ± 0.05) × 1011 M⊙. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | Galaxies: high-redshift | en_US |
| dc.subject | Galaxies: starburst | en_US |
| dc.subject | Submillimetre: galaxies | en_US |
| dc.subject | ALMA survey | en_US |
| dc.subject | SCUBA-2 | en_US |
| dc.title | An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 sub-millimetre galaxies | en_US |
| dc.type | Article | en_US |
